HR 4887
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Crux |
Right ascension | 12h 53m 21.89463s[1] |
Declination | −60° 19′ 46.5630″[1] |
Apparent magnitude (V) | 5.77[2] |
Characteristics | |
Spectral type | B9 Ia[3] |
U−B color index | −0.34[4] |
B−V color index | +0.32[4] |
Variable type | α Cyg?[5] |
Absolute magnitude (MV) | −7.00[8] |
Details Myr | |
6008 | |
Database references | |
SIMBAD | data |
HR 4887 (HD 111904) is a suspected
Location
HR 4887 is one of the brightest members of the NGC 4775 open cluster, better known as the Jewel Box Cluster.[9] It forms the apex of the prominent letter "A" asterism at the centre of the cluster. The cluster is part of the larger Centaurus OB1 association and lies about 8,500 light years away.
The cluster, and HR 4887 itself, is just to the south-east of
Properties
HR 4887 is a B9
In 1958, HR 4887 was reported to be at visual magnitude 6.80 and on this basis is included in the New Catalogue of Suspected Variable Stars with a range of variation of 5.70 - 6.80.[10] No other observer has measured it far from magnitude 5.75, but measurements of known variable class B stars found that HR 4887 is variable by about a tenth of a magnitude. It is thought likely to be an α Cygni-type variable.[5]
References
- ^ S2CID 18759600.
- .
- S2CID 15874925.
- ^ Bibcode:1984A&AS...58..411D.
- ^ S2CID 8783008.
- S2CID 119231169.
- ^ .
- ^ hdl:11336/145136.
- .
- Bibcode:2009yCat....102025S.